空空导弹的一种优化复合控制方案研究

通过研究空空导弹推力矢量和气动复合控制与一般气动控制方式，讨论了新一代近距格斗型空空导弹的一种控制模式，并参照某型导弹的数学模型及有关气动参数对两种控制方式进行了数字仿真。结果表明，在新一代格斗型空空导弹上采用复合控制方式可明显地改善导弹的总体性能。     

基于相位单差精密测速的动态精密单点定位算法

利用相邻历元间的载波相位单差可求得动态载体的高精度三维速度向量,基于此提出了可精确描述载体运动变化的扩展卡尔曼滤波动态精密单点定位算法。该算法克服了高动态条件下采用简化动力学模型可能引起的系统状态描述失实问题,同时还可输出动态载体的精密速度信息。飞机动态试验结果表明,用该算法的动态单点定位结果与TRACK双差解计算互差得到的三维RMS值,平面分量精度优于3cm,高程分量精度优于6cm,速度测量精度可达mm/s级。     

星间自主相对测距中载波相位整周模糊解算方法研究

载波相位整周模糊度解算是利用载波相位进行星间无线电相对距离测量的关键。介绍编队小卫星的工作特点,针对星间相对距离实时、高精度测量的要求,详细阐述利用双频伪码和载波相位观测值解算载波整周模糊度的方法,推导伪码、载波相位测量误差与模糊度解算误差的关系,讨论降低误差的方法。计算机仿真结果表明,该方法可以在单个测量历元获得载波相位整周模糊解算,解算精度与伪码测距精度成正比关系。     

一种快速求解整周模糊度的方法

针对FARA方法搜索整周模糊度组合数比较大,LAMBDA方法需要浮点解精度比较高的缺点,提出一种求解GPS载波相位测量整周模糊度的分步法。用LAMBDA方法搜索出来的整周模糊度作为FARA方法的初始解,进而用FARA方法解算出它的最终解。实验结果表明,该方法能缩短搜索整周模糊度的时间,快速准确地确定整周模糊度。     

微射流技术的原理及其应用

介绍了微射流技术的原理及其初步应用。基于非线性系统的演化对初始条件具有敏感依赖这个事实发展起来的微射流技术，由于与常规持续喷射射流控制方式相比具有许多优点，因而在流动和换热控制应用方面取得明显的效果。并指出，随着研究工作的深入，该项技术还可望用于高马赫数飞行体表面气体流动控制、火箭发动机推力方向控制等。     

Relativistic electrons high doses at International Space Station and Foton M2/M3 satellites

The paper presents observation of relativistic electrons. Data are collected by the Radiation Risk Radiometer-Dosimeters (R3D) B2/B3 modifications during the flights of Foton M2/M3 satellites in 2005 and 2007 as well as by the R3DE instrument at the European Technology Exposure Facility (EuTEF) on the Columbus External Payload Adaptor at the International Space Station (ISS) in the period February 20 – April 28, 2008. On the Foton M2/M3 satellites relativistic electrons are observed more frequently than on the ISS because of higher (62.8°) inclination of the orbit. At both Foton satellites the usual duration of the observations are a few minutes long. On the ISS the duration usually is about 1 min or less. The places of observations of high doses due to relativistic electrons are distributed mainly at latitudes above 50° geographic latitude in both hemispheres on Foton M2/M3 satellites. A very high maximum is found in the southern hemisphere at longitudinal range 0°–60°E. At the ISS the maximums are observed between 45° and 52° geographic latitude in both hemispheres mainly at longitudes equatorward from the magnetic poles. The measured absolute maximums of dose rates generated by relativistic electrons are found to be as follows: 304 μGy h⁻¹ behind 1.75 g cm⁻² shielding at Foton M2, 2314 μGy h⁻¹ behind 0.71 g cm⁻² shielding at Foton M3 and 19,195 μGy h⁻¹ (Flux is 8363 cm⁻² s⁻¹) behind les than 0.4 g cm⁻² shielding at ISS.     

吊挂系统对波瓣混合排气系统气动热力性能影响

为了明确短舱中吊挂系统的堵塞效应对波瓣混合排气系统气动热力性能的影响,采用数值模拟的方法对包含吊挂的混合排气系统进行了定量研究。研究结果表明,受吊挂系统的影响,在波瓣混合排气系统混合段内,存在着一大尺度的回流区,其作用范围随吊挂长度的增加而增加。在性能参数方面,与未考虑吊挂系统时相比,考虑吊挂之后,虽然混合排气系统出口处热混合效率以及推力系数下降很小,最大降幅仅分别为0.017和0.01,但总压恢复系数却显著下降,最大降幅达到了0.03。此外,随着吊挂系统长度的变化,排气系统出口处的热混合效率、总压恢复系数以及推力系数变化幅度小于0.01,变化很小。     

多加速度计振动分离惯性补偿测力技术

为解决在高超声速脉冲风洞中进行大长细比等特殊模型测力实验所面临的惯性补偿问题,笔者提出了多加速度计振动分离惯性补偿方法。这一方法应用在长细比达20 :1 的模型气动力实验中,得到了较为理想的实验结果     

Analysis of total visual and CCD V-broadband observations of Comet C/1995 O1 (Hale-Bopp): 1995–2001

We developed a general method for determination of water production rates from groundbased visual observations and applied it to Comet Hale–Bopp. Our main objective is to extend the method to include total visual magnitude observations obtained with CCD detector and V filter in the analysis of total visual magnitudes. We compare the CCD V-broadband careful observations of Liller [Liller, W. Pre-perihelion CCD photometry of Comet 1995 O1 (Hale-Bopp). Planet. Space Sci. 45, 1505–1513, 1997; Liller, W. CCD photometry of Comet C/1995 O1 (Hale-Bopp): 1995–2000. Int. Comet Quart. 23(3), 93–97, 2001] with the total visual magnitude observations from experienced international observers found in the International Comet Quarterly (ICQ) archive. A data set of ∼400 CCD observations covering about the same 6 years time span of the ∼12,000 ICQ selected total visual magnitude observations were used in the analysis. A least-square method applied to the water production rates, yields power laws as a function of the heliocentric distances for the pre- and post-perihelion phases. The average dimension of the nucleus as well as its effective active area is determined and compared with values published in the literature.     

Modeling and analysis of mover gaps in tubular moving-magnet linear oscillating motors

A tubular moving-magnet linear oscillating motor (TMMLOM) has merits of high efficiency and excellent dynamic capability. To enhance the thrust performance, quasi-Halbach permanent magnet (PM) arrays are arranged on its mover in the application of a linear electro-hydrostatic actuator in more electric aircraft. The arrays are assembled by several individual segments, which lead to gaps between them inevitably. To investigate the effects of the gaps on the radial magnetic flux density and the machine thrust in this paper, an analytical model is built considering both axial and radial gaps. The model is validated by finite element simulations and experimental results. Distributions of the magnetic flux are described in condition of different sizes of radial and axial gaps. Besides, the output force is also discussed in normal and end windings. Finally, the model has demonstrated that both kinds of gaps have a negative effect on the thrust, and the linear motor is more sensitive to radial ones.